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13 October 1986 Diffraction-Limited 10 µm Imaging With 3 Meter Telescopes
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We have constructed an infrared imaging system that achieves diffraction-limited spatial resolution (about 0.8 arc seconds) at 10 um on 3 meter ground-based telescopes. The system uses a linear array of sensitive HgCdTe photodiodes, scanned in the direction perpendicular to the array axis, to form two-dimensional images. Scans are completed rapidly enough to freeze atmospheric fluctuations. Individual detectors are small compared to the diameter of the Airy disk, and images are oversampled heavily in the scan direction. This method has a number of advantages for studying small fields with very high spatial resolution, and has been applied successfully to the problem of directly imaging faint circumstellar dust shells.
© (1986) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
E. E. Bloemhof, C. H. Townes, and A. H. B. Vanderwyck "Diffraction-Limited 10 µm Imaging With 3 Meter Telescopes", Proc. SPIE 0627, Instrumentation in Astronomy VI, (13 October 1986);


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